{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:BVVUCU56A46DRWE6PIRXFN5PX7","short_pith_number":"pith:BVVUCU56","schema_version":"1.0","canonical_sha256":"0d6b4153be073c38d89e7a2372b7afbfec3a619d4b0e5eabedc0b778374913f7","source":{"kind":"arxiv","id":"1411.1431","version":1},"attestation_state":"computed","paper":{"title":"Matching the Evolution of the Stellar Mass Function Using Log-normal Star Formation Histories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"(2) Carnegie Observatories, (3) Padova Astronomical Observatory/INAF, (4) Kavli IPMU), Alan Dressler (2), Augustus Oemler (2), Benedetta Vulcani (4) ((1) UChicago/KICP, Bianca Poggianti (3), Louis E. Abramson (1), Michael D. Gladders (1)","submitted_at":"2014-11-05T22:21:07Z","abstract_excerpt":"We show that a model consisting of individual, log-normal star formation histories for a volume-limited sample of $z\\approx0$ galaxies reproduces the evolution of the total and quiescent stellar mass functions at $z\\lesssim2.5$ and stellar masses $M_*\\geq10^{10}\\,{\\rm M_\\odot}$. This model has previously been shown to reproduce the star formation rate/stellar mass relation (${\\rm SFR}$--$M_*$) over the same interval, is fully consistent with the observed evolution of the cosmic ${\\rm SFR}$ density at $z\\leq8$, and entails no explicit \"quenching\" prescription. We interpret these results/feature"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1411.1431","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-11-05T22:21:07Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"b160491210ebc7cf35e4098b689119e0051a977924f183dd444909e638e043df","abstract_canon_sha256":"a659b8d8cd4c43998135972eefa7bcfb5cfd87adb2738511e0ef05fbc12c744d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:34.613723Z","signature_b64":"DOdNxA+hhxz+194cgVxqJ0tmaoVKotlmFplrsjwqKYgrWjFqsBBlfsv/ttVDssjQcBM1v0M87KfCihAstEFcBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0d6b4153be073c38d89e7a2372b7afbfec3a619d4b0e5eabedc0b778374913f7","last_reissued_at":"2026-05-18T01:41:34.613021Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:34.613021Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Matching the Evolution of the Stellar Mass Function Using Log-normal Star Formation Histories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"(2) Carnegie Observatories, (3) Padova Astronomical Observatory/INAF, (4) Kavli IPMU), Alan Dressler (2), Augustus Oemler (2), Benedetta Vulcani (4) ((1) UChicago/KICP, Bianca Poggianti (3), Louis E. Abramson (1), Michael D. Gladders (1)","submitted_at":"2014-11-05T22:21:07Z","abstract_excerpt":"We show that a model consisting of individual, log-normal star formation histories for a volume-limited sample of $z\\approx0$ galaxies reproduces the evolution of the total and quiescent stellar mass functions at $z\\lesssim2.5$ and stellar masses $M_*\\geq10^{10}\\,{\\rm M_\\odot}$. This model has previously been shown to reproduce the star formation rate/stellar mass relation (${\\rm SFR}$--$M_*$) over the same interval, is fully consistent with the observed evolution of the cosmic ${\\rm SFR}$ density at $z\\leq8$, and entails no explicit \"quenching\" prescription. We interpret these results/feature"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.1431","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1411.1431","created_at":"2026-05-18T01:41:34.613133+00:00"},{"alias_kind":"arxiv_version","alias_value":"1411.1431v1","created_at":"2026-05-18T01:41:34.613133+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.1431","created_at":"2026-05-18T01:41:34.613133+00:00"},{"alias_kind":"pith_short_12","alias_value":"BVVUCU56A46D","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_16","alias_value":"BVVUCU56A46DRWE6","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_8","alias_value":"BVVUCU56","created_at":"2026-05-18T12:28:22.404517+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.21599","citing_title":"JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: stellar population catalogue for galaxies in GOODS-N and GOODS-S","ref_index":268,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BVVUCU56A46DRWE6PIRXFN5PX7","json":"https://pith.science/pith/BVVUCU56A46DRWE6PIRXFN5PX7.json","graph_json":"https://pith.science/api/pith-number/BVVUCU56A46DRWE6PIRXFN5PX7/graph.json","events_json":"https://pith.science/api/pith-number/BVVUCU56A46DRWE6PIRXFN5PX7/events.json","paper":"https://pith.science/paper/BVVUCU56"},"agent_actions":{"view_html":"https://pith.science/pith/BVVUCU56A46DRWE6PIRXFN5PX7","download_json":"https://pith.science/pith/BVVUCU56A46DRWE6PIRXFN5PX7.json","view_paper":"https://pith.science/paper/BVVUCU56","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1411.1431&json=true","fetch_graph":"https://pith.science/api/pith-number/BVVUCU56A46DRWE6PIRXFN5PX7/graph.json","fetch_events":"https://pith.science/api/pith-number/BVVUCU56A46DRWE6PIRXFN5PX7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BVVUCU56A46DRWE6PIRXFN5PX7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BVVUCU56A46DRWE6PIRXFN5PX7/action/storage_attestation","attest_author":"https://pith.science/pith/BVVUCU56A46DRWE6PIRXFN5PX7/action/author_attestation","sign_citation":"https://pith.science/pith/BVVUCU56A46DRWE6PIRXFN5PX7/action/citation_signature","submit_replication":"https://pith.science/pith/BVVUCU56A46DRWE6PIRXFN5PX7/action/replication_record"}},"created_at":"2026-05-18T01:41:34.613133+00:00","updated_at":"2026-05-18T01:41:34.613133+00:00"}